Search Results - "Kunow, H."

STEREO IMPACT Investigation Goals, Measurements, and Data Products Overview by Luhmann, J. G., Curtis, D. W., Schroeder, P., McCauley, J., Lin, R. P., Larson, D. E., Bale, S. D., Sauvaud, J.-A., Aoustin, C., Mewaldt, R. A., Cummings, A. C., Stone, E. C., Davis, A. J., Cook, W. R., Kecman, B., Wiedenbeck, M. E., von Rosenvinge, T., Acuna, M. H., Reichenthal, L. S., Shuman, S., Wortman, K. A., Reames, D. V., Mueller-Mellin, R., Kunow, H., Mason, G. M., Walpole, P., Korth, A., Sanderson, T. R., Russell, C. T., Gosling, J. T.

“…The IMPACT (In situ Measurements of Particles And CME Transients) investigation on the STEREO mission was designed and developed to provide multipoint solar…”
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Solar energetic electrons related to the 28 October 2003 flare by Klassen, A., Krucker, S., Kunow, H., Müller-Mellin, R., Wimmer-Schweingruber, R., Mann, G., Posner, A.

“…We investigate the solar origin of near‐relativistic electrons and protons during the X17.2/4B flare as observed by the Comprehensive Suprathermal and…”
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Ulysses COSPIN observations of cosmic rays and solar energetic particles from the South Pole to the North Pole of the Sun during solar maximum by McKibben, R. B., Connell, J. J., Lopate, C., Zhang, M., Anglin, J. D., Balogh, A., Dalla, S., Sanderson, T. R., Marsden, R. G., Hofer, M. Y., Kunow, H., Posner, A., Heber, B.

“…In 2000–2001 Ulysses passed from the south to the north polar regions of the Sun in the inner heliosphere, providing a snapshot of the latitudinal structure of…”
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Energetic Particle Observations: Report of Working Group C by Klecker, B, Kunow, H, Cane, H V, Dalla, S, Heber, B, Kecskemety, K, Klein, K-L, Kota, J, Kucharek, H, Lario, D, Lee, MA, Popecki, MA, Posner, A, Rodriguez-Pacheco, J, Sanderson, T, Simnett, G M, Roelof, E C

“…Issue Title: Special Issue: Coronal Mass Ejections The characteristics of solar energetic particles (SEP) as observed in interplanetary space provide…”
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Ulysses Cosmic Ray and Solar Particle Investigation/Kiel Electron Telescope observations: Charge sign dependence and spatial gradients during the 1990–2000 A > 0 solar magnetic cycle by Heber, B., Wibberenz, G., Potgieter, M. S., Burger, R. A., Ferreira, S. E. S., Müller-Mellon, R., Kunow, H., Ferrando, P., Raviart, A., Paizis, C., Lopate, C., McDonald, F. B., Cane, H. V.

“…Ulysses, launched in October 1990, began its second out‐of‐ecliptic orbit in September 1997. From 1991 to mid‐2000, solar polar magnetic field observations…”
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Energetic particle observations from the Ulysses COSPIN instruments obtained during the October–November 2003 events by McKibben, R. B., Anglin, J. D., Connell, J. J., Dalla, S., Heber, B., Kunow, H., Lopate, C., Marsden, R. G., Sanderson, T. R., Zhang, M.

“…We report comprehensive observations of solar energetic particle intensities at energies from 0.3 to >100 MeV made by the suite of six Ulysses COSPIN energetic…”
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Energetic Particle Observations by Klecker, B, Kunow, H, Cane, H V, Dalla, S, Heber, B, Kecskemety, K, Klein, K-L, Kota, J, Kucharek, H, Lario, D, Lee, MA, Popecki, MA, Posner, A, Rodriguez-Pacheco, J, Sanderson, T, Simnett, G M, Roelof, E C

“…The characteristics of solar energetic particles (SEP) as observed in interplanetary space provide fundamental information about the origin of these particles,…”
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Evolution of the galactic cosmic ray electron to proton ratio: Ulysses COSPIN/KET observations by Heber, B., Clem, J. M., Müller-Mellin, R., Kunow, H., Ferreira, S. E. S., Potgieter, M. S.

“…The Ulysses orbit provides a unique opportunity to study the propagation of cosmic rays in a wide range of heliographic latitudes and during different solar…”
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Localized “Jets” of Jovian electrons observed during Ulysses’ distant Jupiter flyby in 2003–2004 by McKibben, R.B., Zhang, M., Heber, B., Kunow, H., Sanderson, T.R.

“…We report observations of strongly anisotropic flows of electron events originating from Jupiter that were observed during Ulysses distant Jupiter flyby. A…”
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COSTEP - Comprehensive Suprathermal and Energetic Particle Analyser by Müller-Mellin, R., Kunow, H., Fleißner, V., Pehlke, E., Rode, E., Röschmann, N., Scharmberg, C., Sierks, H., Rusznyak, P., Mckenna-Lawlor, S., Elendt, I., Sequeiros, J., Meziat, D., Sanchez, S., Medina, J., del Peral, L., Witte, M., Marsden, R., Henrion, J.

“…The COSTEP experiment on SOHO forms part of the CEPAC complex of instruments that will perform studies of the suprathermal and energetic particle populations…”
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An overview of Jovian electrons during the distant Ulysses Jupiter flyby by Heber, B., Potgieter, M.S., Ferreira, S.E.S., Dalla, S., Kunow, H., Müller-Mellin, R., Wibberenz, G., Paizis, C., Sarri, G., Marsden, R.G., McKibben, R.B., Zhang, M.

“…Since the 1970's interplanetary electrons in the MeV energy range, of Jovian origin, have been extensively studied from close to the Sun to beyond the Kronian…”
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ICMEs at High Latitudes and in the Outer Heliosphere: Report of Working Group H by Gazis, PR, Balogh, A, Dalla, S, Decker, R, Heber, B, Horbury, T, Kilchenmann, A, Kota, J, Kucharek, H, Kunow, H, Lario, D, Potgieter, MS, Richardson, J D, Riley, P, Rodriguez, L, Siscoe, G, Steiger, R

“…Issue Title: Special Issue: Coronal Mass Ejections Interplanetary coronal mass ejections (ICMEs) propagate into the outer heliosphere, where they can have a…”
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Processes associated with particle transport in corotating interaction regions and near stream interfaces by Intriligator, D. S., Jokipii, J. R., Horbury, T. S., Intriligator, J. M., Forsyth, R. J., Kunow, H., Wibberenz, G., Gosling, J. T.

“…Pioneer and Ulysses observations of energetic particles and solar wind plasma and magnetic fields are analyzed to study particle transport in corotating…”
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Injection and propagation of solar protons to high heliospheric latitudes: Ulysses Ket observations by Struminsky, A., Heber, B., Kallenrode, M.-B., Müller-Mellin, R., Klassen, A., Kunow, H.

“…The Ulysses spacecraft at high heliographic latitudes has detected eight large solar energetic particle events during the recent solar maximum in 2000 and 2001…”
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3-20 MeV Electrons in the Inner Three-dimensional Heliosphere at Solar Maximum: Ulysses COSPIN/KET Observations by Heber, B, Ferrando, P, Raviart, A, Paizis, C, Posner, A, Wibberenz, G, Müller-Mellin, R, Kunow, H, Potgieter, M. S, Ferreira, S. E. S, Burger, R. A, Fichtner, H, Schlickeiser, R

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ICMEs at High Latitudes and in the Outer Heliosphere by Gazis, PR, Balogh, A, Dalla, S, Decker, R, Heber, B, Horbury, T, Kilchenmann, A, Kota, J, Kucharek, H, Kunow, H, Lario, D, Potgieter, MS, Richardson, J D, Riley, P, Rodriguez, L, Siscoe, G, Steiger, R

“…Interplanetary coronal mass ejections (ICMEs) propagate into the outer heliosphere, where they can have a significant effect on the structure, evolution, and…”
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Role of low-frequency modes in organizing the inner heliosphere by Heinen, Oliver, Lanzerotti, Louis J., Heber, B., Kunow, H., Thomson, David J.

“…Cosmic ray proton data (125 to >2000 MeV) measured in the inner three‐dimensional (3‐D) heliosphere over the years from 1993 into 2000 by the KET instrument on…”
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Amplitude evolution and rigidity dependence of the 26-day recurrent cosmic ray decreases: COSPIN/KET results by Paizis, C., Heber, B., Ferrando, P., Raviart, A., Falconi, B., Marzolla, S., Potgieter, M. S., Bothmer, V., Kunow, H., Müller‐Mellin, R., Posner, A.

“…In the time interval extending from July 1992 to July 1994, Ulysses climbed from 10°S heliographic latitude up to over 70°S. During this time lapse, solar…”
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The Ulysses fast latitude scans: COSPIN/KET results by Heber, B., Sarri, G., Wibberenz, G., Paizis, C., Ferrando, P., Raviart, A., Posner, A., Müller-Mellin, R., Kunow, H.

“…Ulysses, launched in October 1990, began its second out-of-ecliptic orbit in December 1997, and its second fast latitude scan in September 2000. In contrast to…”
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Differences in the temporal variations of galactic cosmic ray electrons and protons: Implications from Ulysses at solar minimum by Heber, B., Ferrando, P., Raviart, A., Wibberenz, G., Müller-Mellin, R., Kunow, H., Sierks, H., Bothmer, V., Posner, A., Paizis, C., Potgieter, M. S.

“…According to standard drift dominated modulation models the intensity variations of galactic cosmic ray protons and electrons respond differently to the…”
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